Abstract The Electric and Magnetic Field Instrument and Integrated Science (EMFISIS)
investigation on the NASA Radiation Belt Storm Probes (now named the Van Allen Probes) …

Earth's radiation belt electrons exhibit pronounced dynamic variability in response to solar
activity and resultant changes in the solar wind. The nonadiabatic variability of radiation belt …

The flux of energetic electrons in the Earth's outer radiation belt can vary by several orders of
magnitude over time scales less than a day, in response to changes in properties of the …

Earth's diffuse aurora occurs over a broad latitude range and is primarily caused by the
precipitation of low-energy (0.1–30-keV) electrons originating in the central plasma sheet …

Pulsating aurora, a spectacular emission that appears as blinking of the upper atmosphere
in the polar regions, is known to be excited by modulated, downward-streaming electrons …

Gyroresonant wave particle interactions with whistler mode chorus play a fundamental role
in the dynamics of the Earth's radiation belts and inner magnetosphere, affecting both the …

Whistler mode chorus waves are receiving increased scientific attention due to their
important roles in both acceleration and loss processes of radiation belt electrons. A new …

The flux of relativistic electrons in the Earth's radiation belts is highly variable and can
change by orders of magnitude on timescales of a few hours. Understanding the drivers for …

Using the statistical wave power spectral profiles obtained from CRRES wave data within
the 0000–0600 MLT sector under different levels of geomagnetic activity and a modeled …

A statistical survey of plasma densities and electron distributions (0.5–100 keV) is performed
using data obtained from the Time History of Events and Macroscale Interactions During …